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Semiempirical approximations elements

The reason we employ two rather distinct methods of inquiry is that neither, by itself, is free of open methodological issues. The method of molecular dynamics has been extensively applied, inter alia, to cluster impact. However, there are two problems. One is that the results are only as reliable as the potential energy function that is used as input. For a problem containing many open shell reactive atoms, one does not have well tested semiempirical approximations for the potential. We used the many body potential which we used for the reactive system in our earlier studies on rare gas clusters containing several N2/O2 molecules (see Sec. 3.4). The other limitation of the MD simulation is that it fails to incorporate the possibility of electronic excitation. This will be discussed fmther below. The second method that we used is, in many ways, complementary to MD. It does not require the potential as an input and it can readily allow for electronically excited as well as for charged products. It seeks to compute that distribution of products which is of maximal entropy subject to the constraints on the system (conservation of chemical elements, charge and... [Pg.67]

Semiempirical Approximation. The method that adopts a semiempirical approximation to a uses the Andersen-Hinthome local thermodynamic equilibrium (LTE) model [185] for estimating the degree of ionization. The model does not take account of any details of individual ionization processes but assumes that the region at and near the surface involved in sputtering can be approximated by a dense plasma in local thermodynamic equilibrium. The plasma has an associated temperature T. The ratio of the concentrations of two elements X and Y in a matrix B, if sufficiently dilute, can then be written as... [Pg.895]

Once the format of the Fock matrix is known, the semiempirical molecular problem (and it is a considerable one) is finding a way to make valid approximations to the elements in the Fock matrix so as to avoid the many integrations necessary in ab initio evaluation of equations like Fij = J 4>,F4> dx. After this has been done, the matrix equation (9-62) is solved by self-consistent methods not unlike the PPP-SCF methods we have already used. Results from a semiempirical... [Pg.279]

We now turn to the problem of simplifying the recovery of the dynamic correlation energy. We consider the simplest situation, viz., where the zeroth-order wavefunction can be chosen as the SCF approximation. A challenging disparity exists between the energetic smallness of these refinements and the complexity and magnitude of the computational efforts required for their variational determination. In order to reduce this disproportion, various semiempirical approaches have been proposed (56-61), notably in particular the introduction of semiempirical elements into MP2 theory which has led to the successful Gn methods (62-64). [Pg.114]

In that study [31], we estimated the electronic coupling with the help of HF/6-31G calculations. Any attempt to expand such an investigation into a reasonably quantitative description of the variation of the electronic coupling over time would be much too costly. As noted above, one can overcome that problem by constructing a special semiempirical method (e.g., NDDO-HT) affording sufficiently accurate estimates of electronic matrix elements, or by using an approximate relation between H a and the overlap of related orbitals. [Pg.68]

Numerous other semiempirical methods have been proposed. The MNDO method has been extended to d functions by Theil and coworkers and is referred to as MNDO/d.155>156 For second-row and heavier elements, this method does significantly better than other methods. The semi-ab initio method 1 (SAM1)157>158 is based on the NDDO approximation and calculates some one- and two-center two-electron integrals directly from atomic orbitals. [Pg.183]

Fig. 6.1 The principle behind the semiempirical calculation of heat of formation (enthalpy of formation). The molecule is (conceptually) atomized at 298 K the elements in their standard states are also used to make these atoms, and to make the molecule M. The heat of formation of M at 298 K follows (with some approximations) from equating the energy needed to generate the atoms via M to that needed to make them directly from the elements... Fig. 6.1 The principle behind the semiempirical calculation of heat of formation (enthalpy of formation). The molecule is (conceptually) atomized at 298 K the elements in their standard states are also used to make these atoms, and to make the molecule M. The heat of formation of M at 298 K follows (with some approximations) from equating the energy needed to generate the atoms via M to that needed to make them directly from the elements...
J.J.P. Stewart, Optimization of parameters for semiempirical methods V Modification of NDDO approximations and application to 70 elements. J. Mol. Model. 13, 1173-1213 (2007)... [Pg.213]

The highly specific behavior of transition metal complexes has prompted numerous attempts to access this Holy Grail of the semi-empirical theory - the description of TMCs. From the point of view of the standard HFR-based semiempirical theory, the main obstacle is the number of integrals involving the d- AOs of the metal atoms to be taken into consideration. The attempts to cope with these problems have been documented from the early days of the development of semiempirical quantum chemistry. In the 1970s, Clack and coworkers [78-80] proposed to extend the CNDO and INDO parametrizations by Pople and Beveridge [39] to transition elements. Now this is an extensive sector of semiempirical methods, differing by expedients of parametrizations of the HFR approximation in the valence basis. These are, for example, in methods of ZINDO/1, SAMI, MNDO(d), PM3(tm), PM3 etc. [74,81-86], From the... [Pg.122]

This is the simplest possible mechanistic model of the PES, derived from an approximate treatment of energy according to eq. (3.69). The FA type of treatment implies that the geminal amplitude-related ES V eqs. (2.78) and (2.81) are fixed at their invariant values eq. (3.7). This corresponds clearly to a simplified situation where all bonds are single ones. Within such a picture, the dependence of the energy on the interatomic distance reduces to that of the matrix elements of the underlying QM (MINDO/3 or NDDO) semiempirical Hamiltonian. [Pg.231]

Specificity of any semiempirical parametrization is that in the FA approximation the one-center energies Ea eq. (2.88) related to the carbon atom remain hybridization-independent (see below and [44] and [45]). This result which ultimately comes from the fact that in carbon the valence shell is half filled, distinguishes carbon among other elements. For that reason (in the FA approximation) only the resonance contribution to the total energy depends both on orientation (as in the FAFO model) and on the form of the hybridization tetrahedra. This considerably simplifies the derivation in the case of carbon atoms. For that reason we consider it separately. [Pg.241]

In general, CNDO/2, INDO, and PRDDO mimic ab initio results by artful and compensating approximations and semiempirical parameters, and they yield reasonable dipole moments and charge distributions. INDO and ZINDO parameterizations are available for relatively many elements in the periodic table, but their predictions can deviate considerably from experiment. [Pg.176]

Other complications are associated with the partitioning of the core and valence space, which is a fundamental assumption of effective potential approximations. For instance, for the transition elements, in addition to the outermost s and d subshells, the next inner s and p subshells must also be included in the valence space in order to accurately compute certain properties (54). A related problem occurs in the alkali and alkaline earth elements, involving the outer s and next inner s and p subshells. In this case, however, the difficulties are related to core-valence correlation. Muller et al. (55) have developed semiempirical core polarization treatments for dealing with intershell correlation. Similar techniques have been used in pseudopotential calculations (56). These approaches assume that intershell correlation can be represented by a simple polarization of one shell (core) relative to the electrons in another (valence) and, therefore, the correlation energy adjustment will be... [Pg.160]

Equation (54) is the basis for the semiempirical methods to be discussed below. Several approximations have been used for (rXi). In all of the methods, the matrix elements of Hso are evaluated with respect to a wave function variationally optimized in A-S coupling. The spin-orbit matrix is then diagonalized for the various values of the total angular momentum of the system. [Pg.165]

Semiempirical spin-orbit operators play an important role in all-electron and in REP calculations based on Co wen- Griffin pseudoorbitals. These operators are based on rather severe approximations, but have been shown to give good results in many cases. An alternative is to employ the complete microscopic Breit-Pauli spin-orbit operator, which adds considerably to the complexity of the problem because of the necessity to include two-electron terms. However, it is also inappropriate in heavy-element molecules unless used in the presence of mass-velocity and Darwin terms. [Pg.179]

Semiempirical techniques are the next level of approximation for computational simulation of molecules. Compared to molecular mechanics, this approach is slow. The formulations of the self-consistent field equations for the molecular orbitals are not rigorous, particularly the various approaches for neglect of integrals for calculation of the elements of the Fock matrix. The emphasis has been on versatility. For the larger molecular systems involved in solvation, the semiempirical implementation of molecular orbital techniques has been used with great success [56,57]. Recent reviews of the semiempirical methods are given by Stewart [58] and by Rivail [59],... [Pg.233]

In this class of compounds, there are many interesting properties whose solutions, using approximate wave functions, may yield sufficiently accurate results to permit interpretation of the desired phenomena. For this reason we have performed calculations using the semiempirical extended Hiickel method, modified to include a seemingly more justifiable physical interpretation of the matrix elements as well as iterative processes which introduce a measure of self-consistency. We shall discuss this method in detail later, present some results of the calculations, and show their good agreement with experimental results. [Pg.15]

A semiempirical correlation among coupling matrix elements and crossing distances for many molecules was examined by Olson, Smith and Bauer ( ) and Olson (28). The coupling matrix elements calculated from their semiempirical formula agree with our values to within a factor of two, which is not surprising for such an approximate correlation. [Pg.248]


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Semiempirical approximations

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